Solar thermal decomposition of zinc oxide: An initial investigation of the recombination reaction in the temperature range 1100-1250 K

M. Keunecke, A. Meier, R. Palumbo

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44 Scopus citations

Abstract

We present an experimental and theoretical study that explores the zinc vapour and O2 reaction under laminar flow conditions similar to those that may exist at the exit of a high temperature solar reactor used to decompose ZnO(s). The zinc vapour and O2 reaction was experimentally studied in an electrically heated tubular furnace. A finite difference mass transfer model for laminar flow, which accounts for radial diffusion of the gases to the tube wall, was developed to help interpret the experimental results. We found that when the gas and wall temperatures are below the decomposition temperature of ZnO(s) but above the condensation temperature of Zn(g), the mass transfer rate of Zn(g) and O2 to the reactor wall limits the oxidation rate of Zn(g). ZnO(s) decomposition experiments were also carried out in a concentrating solar furnace in order to establish the importance of the temperature of an inert gas used in a solar reactor on the zinc yield. We found that the gas temperature should be above the Zn(g) condensation temperature in the hot region of the reactor in order to avoid oxidation of zinc vapour before it enters the quench unit.

Original languageEnglish (US)
Pages (from-to)2695-2704
Number of pages10
JournalChemical Engineering Science
Volume59
Issue number13
DOIs
StatePublished - Jul 2004
Externally publishedYes

Bibliographical note

Funding Information:
Financial support by the Swiss Federal Office of Energy is gratefully acknowledged. The authors also thank J. Lédé and M. Ferrer from CNRS-ENSIC Nancy, France, for discussions with regard to the presentation and interpretation of experimental results obtained in the Solar Furnace, Paul Scherrer Institut, Villigen, Switzerland.

Keywords

  • Mass transfer modelling
  • Oxidation of zinc vapour
  • Production of Zn(s) from ZnO(s)
  • Quenching
  • Solar fuels
  • Solar thermal chemistry

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